Interactions in massive binary stars as seen by interferometry
arXiv:1201.1651 · doi:10.1007/978-3-642-30648-8_5
Abstract
With the advent of large-collecting-area instruments, the number of objects that can be reached by optical long-baseline interferometry is steadily increasing. We present here a few results on massive binary stars, showing the interest of using this technique for studying the insight of interactions in these systems. Indeed, many massive stars with extended environments host, or are suspected to host, companion stars. These companions could have an important role in shaping the circumstellar environment of the system. These examples provide a view in which binarity could be an ingredient, among many others, for the activity of these stars.
From solar environment to stellar environment, Roscoff : France (2011)
References in corpus (11)
- Effects of gravitational darkening on the determination of fundamental parameters in fast rotating B-type stars
- First spectro-interferometric survey of Be stars I. Observations and constraints on the disks geometry and kinematics
- Gas Distribution, Kinematics, and Excitation Structure in the Disks around the Classical Be Stars Beta Canis Minoris and Zeta Tauri
- An asymmetry detected in the disk of Kappa CMa with the AMBER/VLTI
- The 2011 outburst of the recurrent novaT Pyx. Evidence for a face-on bipolar ejection
- VLTI monitoring of the dust formation event of the Nova V1280 Sco
- A silicate disk in the heart of the Ant
- A disc in the heart of the Ant nebula
- The close-in companion of the fast rotating Be star Achernar
- delta Cen: a new binary Be star detected by VLTI/AMBER spectro-interferometry
- X-ray Emission from Magnetically Torqued Disks of Oe/Be Stars